Hadronic high-energy gamma ray emission from microquasars

dc.creatorRomero, Gustavo Esteban
dc.creatorChristiansen, Hugo
dc.creatorOrellana, Mariana Dominga
dc.date.accessioned2017-12-07T14:52:41Z
dc.date.accessioned2018-11-06T15:55:36Z
dc.date.available2017-12-07T14:52:41Z
dc.date.available2018-11-06T15:55:36Z
dc.date.created2017-12-07T14:52:41Z
dc.date.issued2005-06
dc.identifierRomero, Gustavo Esteban; Christiansen, Hugo; Orellana, Mariana Dominga; Hadronic high-energy gamma ray emission from microquasars; IOP Publishing; Astrophysical Journal; 632; 6-2005; 1093-1098
dc.identifier0004-637X
dc.identifierhttp://hdl.handle.net/11336/29928
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1902530
dc.description.abstractWe present a hadronic model for gamma-ray production in the microquasar LS I +61 303. The system is formed by a neutron star that accretes matter from the dense and slow equatorial wind of the Be primary star. We calculate the gamma-ray emission originating from pp interactions between relativistic protons in the jet and cold protons from the wind. After taking into account opacity effects on the gamma rays introduced by the different photon fields, we present high-energy spectral predictions that can be tested with the new-generation Cerenkov telescope MAGIC.
dc.languageeng
dc.publisherIOP Publishing
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1086/444446
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2005ApJ...632.1093R
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectGamma rays
dc.subjectHadrons
dc.subjectMicroquasars
dc.subjectLS I +61 303 (microcuásar)
dc.titleHadronic high-energy gamma ray emission from microquasars
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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